Physics · Unit 3 · Gravity and motion · Projectile motion

Solve vector problems by resolving vectors into components, adding or subtracting the components and recombining them to determine the resultant vector.

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Solve problems involving the third law of planetary motion using 𝑇𝑎2 𝑟𝑎3 = 𝑇𝑏 2 𝑟𝑏 3 = 4𝜋2 𝐺𝑀. The following subject matter may be assessed in the internal assessments.
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State the three laws of planetary motion.
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